TITLE: GCN CIRCULAR NUMBER: 36489 SUBJECT: GRB 240511A: radio detection of afterglow candidate DATE: 24/05/15 18:05:58 GMT FROM: Lauren Rhodes at Oxford <lauren.rhodes@physics.ox.ac.uk> Lauren Rhodes, Rob Fender (Oxford), Dave Green, Dave Titterington (Cambridge) report: We observed the field of GRB 240511a (GCN 36428, 36430) with the Arcminute Microkelvin Imager - Large Array (AMI-LA) at 15.5 GHz beginning at UT 04:33:54 on 15-May-2024 for a total of 4 hours. The flux standard 3c286 was used to calibrate the bandpass response and flux scale of the AMI-LA and J2232+1143 was used as an interleaved complex gain calibrator. We detected an unresolved radio source at the position of the afterglow candidate (GCN 36442) with a flux density of about 600uJy/beam. The rms noise in the field is about 70uJy/beam. More observations are planned. We thank the staff at the Mullard Radio Astronomy Observatory for carrying out these observations and operating the AMI-LA. View this GCN Circular online at https://gcn.nasa.gov/circulars/36489. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0LW...